Astronomy:110 Virginis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Virgo |
| Right ascension | 15h 02m 54.03756s[1] |
| Declination | +02° 05′ 28.6957″[1] |
| Apparent magnitude (V) | 4.40[2] |
| Characteristics | |
| Evolutionary stage | red clump[3] |
| Spectral type | K0.5 IIIb Fe–0.5[4] |
| B−V color index | 1.04[2] |
| Astrometry | |
| Radial velocity (Rv) | −16.2±0.3[1] km/s |
| Proper motion (μ) | RA: −55.569[1] mas/yr Dec.: +13.628[1] mas/yr |
| Parallax (π) | 16.7474 ± 0.129[1] mas |
| Distance | 195 ± 2 ly (59.7 ± 0.5 pc) |
| Details | |
| Mass | 1.67[2] M☉ |
| Radius | 13.78±0.14[5] R☉ |
| Luminosity | 80.4±1.8[5] L☉ |
| Surface gravity (log g) | 2.7[6] cgs |
| Temperature | 4,655±24[5] K |
| Metallicity [Fe/H] | −0.3[6] dex |
| Age | 4.52[2] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
110 Virginis is a star in the zodiac constellation Virgo, located 195[1] light-years away from Earth. It is visible to the naked eye as an orange-hued star with an apparent visual magnitude of 4.40.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.[1]
The stellar classification of 110 Virginis is K0.5 IIIb Fe–0.5,[4] indicating that this is an evolved giant star with a mild underabundance of iron in its spectrum. At the age of 4.5[2] billion years old, it belongs to a sub-category of giants called the red clump, which means it is on the horizontal branch and is generating energy through the helium fusion at its core.[3] Compared to the Sun, it has 167%[2] of the mass but has expanded to 14 times the size. The enlarged photosphere has an effective temperature of 4,655 K and is radiating 80 times the Sun's luminosity.[5]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal 150 (3): 88, doi:10.1088/0004-6256/150/3/88, Bibcode: 2015AJ....150...88L.
- ↑ 3.0 3.1 Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal 539 (2): 732–741, doi:10.1086/309278, Bibcode: 2000ApJ...539..732A.
- ↑ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K
- ↑ 5.0 5.1 5.2 5.3 Baines, Ellyn K.; Thomas Armstrong, J.; Clark, James H.; Gorney, Jim; Hutter, Donald J.; Jorgensen, Anders M.; Kyte, Casey; Mozurkewich, David et al. (2021), "Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer", The Astronomical Journal 162 (5): 198, doi:10.3847/1538-3881/ac2431, Bibcode: 2021AJ....162..198B
- ↑ 6.0 6.1 Hekker, S.; Meléndez, J. (December 2007), "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters", Astronomy & Astrophysics 475 (3): 1003–1009, doi:10.1051/0004-6361:20078233, Bibcode: 2007A&A...475.1003H.
- ↑ "110 Vir". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=110+Vir.
Coordinates: 
15h 02m 54.0s, +02° 05′ 28.7″
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